From the Director





by Rex Parker, Director

Members Night at Observatory Saturday, June 16. Hoping third time is a charm after clouds and rain washed us out on May 12 and May 19. Mark your calendar for a Members Night (and family and friends too) at AAAP’s Observatory in Washington Crossing Park on June 16. See the website for info on how to get there (phone 737-2575). Sunset on June 16 is ~8:30 pm, so come around then if you want to see the thin crescent moon, or anytime after till at least midnight.

If you’re a newer member or haven’t been out there for a while, you may be amazed to see the latest equipment in action. The Mallincam video camera has been retired to make way for new technology, including a Starlight Xpress Ultrastar-C color CCD camera on a 5” Explore Scientific apochromatic refractor, and a ZWO ASI-294 color CMOS camera on a 10” Mewlon Cassegrain reflector scope. These are in addition to the Celestron-14 and the legendary 1879 Hastings 6-1/4” refractor set up for visual observing with eyepieces. All telecopes slew around the sky robotically on Software Bisque Paramount equatorial mounts. For more on planetary viewing opportunities next month see below.

Martian Insight. While Jupiter still dominates the southern night sky this month, Mars will brighten rapidly in June and outshine the Jovian planet by the end of July as it reaches perihelic opposition. That means it lies opposite to the sun in our sky, and while this happens every other earth year, the closeness varies from eccentricity in the orbit over the 687 earth day orbital period of Mars (Martian year). This summer Mars will be within 36 million miles of earth, the closest it’s been since summer of 2003. I went back to the archives on my home PC and found these images (below) I took at the 2003 opposition, using a 5” refractor with barlow to give a focal ration of f/40.

Jun 16 (EDT) Rise time & azimuth Transit time & altitudeK/th>

Magnitude Diameter, arcsec
Mars 23:23 119 04:10 28S -1.7 18
Jupiter 16:57 109 22:07 35S -2.4 43
Saturn 21:06 119 01:51 27S 0.1 18

These color images were made from separate subframes using an SBIG ST10 CCD camera with red, green, and blue filters, a much more difficult technique than using the new “one-shot color” cameras at the Observatory. The key to planetary imaging is to take many brief frames in order to capture the best ones at those occasional instants of atmospheric clarity. The new cameras have high sensitivity and very fast download rates allowing them to be used (with the right software) as streaming color video or to capture individual frames. The control software (“Starlight Live” and “SharpCap”; read about these online) is reasonably intuitive. It’s hoped that AAAP members will enjoy using these cameras to photograph planets, moon, and deep sky objects. Feel free to contact me or the Observatory or Outreach Chairs if you have questions about use (see the Contact Us tab on the website).

Seeking deeper impressions of Mars, the NASA Mars Insight mission launched successfully a few weeks ago (). The Insight craft is now in interplanetary space bound for Mars. Science instruments on board are designed to measure the interior geophysics of the red planet, including a seismometer and a thermal conductivity probe. The anticipated data will help develop better understanding of how Mars apparently lost its magnetic field in its distant past. If successful the measurements will also provide insight into previous plate tectonic activity and help drive hypotheses on how and when Mars may have lost it’s original atmosphere and water. Deep questions in need of answers!

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From the Program Chair

By Ira Polans

The June meeting of the AAAP, and our last until next September, will take place on June 12th at the in Trenton. The meeting starts at 7:30 PM.

In addition to our normal club meeting, attendees will view the latest show “Dark Universe”. Narrated by astrophysicist Neil deGrasse Tyson, the show celebrates a new age of cosmic discovery as well as its deepest mysteries. Dark Universe features spectacular scenes of recent spacecraft, such as the Galileo probe’s breathtaking plunge into Jupiter’s atmosphere, the most accurate visualizations ever produced, such as a Milky Way galaxy spangled with exploding supernovas, and novel renderings of hotly discussed phenomena, like dark matter.

There is plenty of parking in front of the planetarium entrance behind the museum. Museum is located at –205 W. State Street, Trenton, NJ 08625.

We look forward to seeing you at the meeting.

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From the Outreach Chair

Gene Allen, Outreach Chair

Upcoming Outreach Events

Response to requests for AAAP member support has recently blossomed. We have good numbers for our Solar Observation session, held annually at the Nature Center on Memorial Day weekend and jointly with Washington Crossing State Park. We have outstanding support for opening the Observatory to Scouts on a Saturday, and I hope members will step up in equal or greater numbers for the Hopewell event later in June.

In order to clearly divide responsibilities, we consider any requests for use of the observatory on other than Friday Public Nights, and for Public Night attendance by any group numbering twenty or more, to constitute an Outreach Event. Appeals for support for these events, as well as events at schools and other off-site locations, are conducted by Outreach. These events are entered into the AAAP website calendar, including as much detail about location and group size and age as are available. Names of those who volunteer are added as they step up, but if your name gets neglected, be sure to holler! PLEASE GET INTO THE HABIT OF CHECKING THE CALENDAR OFTEN! Revisions to the website explaining these details are admittedly overdue but have not yet been submitted. Work installing lighting and new cameras in the Observatory have been diverting…

Any members who wish to participate specifically in Outreach Events, and be part of the Outreach Committee, please email. This will not obligate you to every event, but you will be included in the first appeal and have more of a voice in the handling of Outreach Events.

These are the two upcoming Outreach Events on the schedule for June, as copied from the calendar. The calendar entry for the Hopewell event also includes location details.

Saturday, June 9
Cub Scout Pack 44 of Pennington will be camping in WCSP over Saturday night and have asked us to open Simpson Observatory for a total of about 30 Cub Scouts, Boy Scouts, and parents. We will not be open to the general public, so the gates will be reclosed after volunteers enter, and any non-Keyholder Members will need to coordinate entry. Volunteers so far are Tim Donney, Jen & Dave Skitt, Tom Swords, Jim Fling, Luisa & Tim Gong, and Ira Polans. These are all Keyholders so we are indeed well covered, thank you! An Outreach Member bringing an additional scope is David Letcher.

Saturday, June 23
Some 45 families totaling 200 people are expected to participate in the Hopewell Community Campout. AAAP has been asked to bring scopes and binoculars, setting up in advance between the picnic table and the campfire (see attached map) to support a “nature at night” program planned to run from dark for about an hour.


Volunteers so far include Dave Reis and Tim Donney.

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May 8, 2018 Meeting Minutes

by Jim Poinsett, Secretary

Minutes of the May 8, 2018 of the Amateur Astronomers Association of Princeton

  • Director Rex Parker called the meeting to order and called upon the nominating committee to run the election of the board of directors. The entire current board was nominated to return and were elected unanimously.
  • Bill Murray gave a 10 minute talk on Stellafane, the “Shrine to the Stars”. It is the oldest gathering of amateur astronomers in the United States. It is held annually on the new moon weekend in July or August.
  • New keyholder Scott Smith received his key.
  • Gene reported that two new cameras were acquired at NEAF and will be installed as soon as possible. Also purchased was an adapter to align the Mewlon with the HB refractor.
  • Outreach reported that a scout group will be at the observatory on June 9th. Volunteers are needed as it will be a sizeable group.
  • The possibility of family memberships was discussed and will be discussed at a future board meeting.
  • It was discovered that Gene Ramsey’s son, Michael, now works for park maintenance. It’s good to have a friend working at the park.
  • Next meeting is at the planetarium at the NJ State Museum in Trenton.
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momma’s red shoe

by Ted Frimet

momma’s red shoe


It wasn’t too long ago when I joined an astronomy forum, at Google+. And yes, the name of the forum is “Astronomy”. Therein lay over 24,000 members; of which there are a dozen contributors during any given week. Most recently, Astronomy forum member Andleeb Atal posted his brief on the “Wow” signal, acknowledged by an Ohio States University telescope program, of August 15, 1977. Astronomer Antonio Paris at Florida’s St. Petersburg College attributed the signal to comet 266P Christensen. He included a second comet possibility, named P/2008 Y Gibbs. Neither long-haired beasty was known to be in existence, in 1977. You will get no argument from me, here, on the time-line.

What I found interesting, is the baseline signal of 1420 Mhz. That is the spectral center line for elemental Hydrogen. Atal notes that were some small discrepancies, noted between the signal residing at 1420.36 (JD Kraus) and 1420.46 (JR Ehman). However, there it hovers at the midline. I would like to lay claim that this side-note became the foundation of new thought, for me; however I would by dying, if not lying about it. Hydrogen, as the most abundant element in the universe, is significantly interesting, all by its lonely self.

What is truly an engaging fact is that not all hydrogen resonates the same way. (doppler shifts -Wikipedia accessed May 7, 2018 8:57 AM) There is truly a very small amount of our universal norm that beats to the tune of 1420 Mhz (mean lifetime of the excited state of around 10 million years; Wikipedia, ibid). Sufficiently so, we are able to listen to it, among the static of the cosmic background radiation. Its hum competes with all sorts of interesting aural phenomenon. Listening to that key chord keeps us sane while existing on our lonely intelligent rock. It is the pervasive thought that life, extraterrestrial intelligent life, will use the universal baseline to pulse encode a message. Comets be damned, we are still searching for a intergalactic dance partner. Shall we dance?

Within the confines of the forum’s articulation, I found myself being perceived as challenging the speed of light. Albert, we will have none of that now. You let over 30 years transpire, while searching to combine electromagnetism with gravity; and appeared to look the other way while Cosmology and Astrophysics unknowingly raced by you. Out of deep respect for a person who simply did not let a thought go by for decades, I will continue to honor the time long tradition of accepting that c is a constant, no matter and where ever you are.

However, some have confused the immutable speed of light with invariant frequency and wavelength. Perhaps this stems from a misunderstanding that pulse encoded messages will not be the same in everyone’s space-time. Forgive me the math mistakes; however you will get to the crux of the idea, right now. If you would, here is what I had to inquire onto my forum participants. Unlike questions, they were more akin to answers.

If the initiator of a signal was in a region of dilated space-time, then their clocks would run at a different rate than ours. For arguments sake, how about twice as slow?

Their counts, per unit time, would be the same as ours. That is, both would be 1420 (Mhz). However, when you stack both transmissions up against each other, one is dilated, one is contracted.

When we receive their baseline broadcast, compared to our local clock, we would have to look for a mid-line of twice Hydrogen (2840 Mhz).

Galaxies, and the stars constrained within, are in motion. And yes, they would need to be moving at speeds close to the light speed, in order for relativity to matter.

However, I am not so sure that space-time is so neat, as to not be [held] accountable for a many clocks theory.

Time passes, and question and answers come and go. Without ado, I am repelled by commentary on Occam’s razor, combined with a coup de grace on not accepting a non-uniformity in space tension. Yes, space-time is tough as an ox. It has the strength several hundred times that of a bar of steel. After receiving the first observation of gravity waves, on September 14, 2015 – we conclude that it took 63 solar masses of two black holes to coalesce and release 3 solar masses of energy to cataclysmically distort space. Yet, I deny neither my fellow commentator invoking Occam, or uniformity in space tension. c prevails, here, untouched. Yet, there is the last question, reserved for the reader who does not know how to ask. In cosmological musing, I offered it below:

I agree. c probably stays the same. Of course, if the medium slows down light; other matter not similarly affected will outpace light in that medium. [cherenkoff radiation].

Here are some notes, I just finished taking a few minutes ago. It manages to mess up the idea that time clocks are not universal; as it related to Einstein over 100 years ago – and still stands correct, today.

Here ya go – I was having an email conversation with our MathFromtheGut, guy:

I was reading and commenting, this morning, on the Hydrogen spectrum line, 1420 Mhz, and how we anticipate intelligent beings to use it as a carrier wave.

My additional comment was relativity related; spatial dilation affects clocks; so 1420 ticks per unit second, there, isn’t my 1420 ticks per unit second, here.

If the clock were twice as slow, I’d imagine my carrier wave to be at 2840 Mhz.

Anyway, stars and galaxies (red-shift aside) are moving at high velocity. Of course I beg the question that they are not moving at light speed.

However, any velocity difference, away or towards us, does compromise a clock, even if slightly.

Then, if we were to look at our common 1420 Mhz (1420.0000) if would be more relativistic to look at 1420.0314; depending on the velocity difference.

Electromagnetic pressure (solar pressure) will increase if the source galaxy velocity is greater.

EM(pressure inc) = Galaxy(v inc) = Gravity(G inc)

Ok. Time for a night cap coffee.

Let me know where this falls apart.

It didn’t fall too far. It held together like the very fabric of space-time. Thor’s hammer couldn’t budge it. It would take collisions of vastly superior astronomical beings to undo Einstein and his building blocks of Faraday, Henry and the treatise of James Clerk Maxwell. And then we return to the opening thrust; the tip of the spear. The Wow signal of 1977, whose base frequency was reported, as two numbers. Now that we have separated the chaff from the wheat, we can now know Wow! for what it is.

A space time dilation effect of 0.00704022% difference

It is a fair supposition that the Wow! signal was initiated from Sagittarius. That much seems to be written in stone. In an effort to avoid an observer paradox in resolving the two observed frequency signatures, I am agreeing that both observed signals came from the same sky region. Aka the same source.
I am adding my hallmark that the signal was split, by the likes of gravitational lensing. This is less mysterious, and it is very compelling. Having the same signal take two paths, and arriving on two different frequencies provides the test bed for a Lorentz transform for time [or distance]. That is, according to either observer, the same signal was received; however on two different frequencies.
I have a radio signal, that passes thru a region in space that splits the signal. One path goes thru “normal” space-time. The other goes thru “time-dilation” – let’s say its clock slows down. However, due to “c” being a constant, both signals arrive at the radio receiver, at the same “time”. The frequencies have shifted by 0.1 Mhz. Show the dilation effect, using Lorentz Transforms. Yup, there’s an app for that. It’s YouTube’s Fermi Lab Presents: “Relativity: how people get time dilation wrong”. Substituting frequency for time in a Lorentz Transform:

V2 = 1/lambda * V1 for our second, time dilated frequency
V2 = lambda * V1 for our first, non-time dilated frequency

Normally viewed, the Lorentz Transforms would be for two different observers. One moving relative to the other. In my special, frequency shifting world, my signals are observing the radios. Yeah, Neo, that will really bake your noodle. Here, have a cookie, and you will be right as rain! Time dilation and length contraction are both side effects of moving thru a regions of space that have different gravity for either of our two signals. (YouTube video: “Travel into the Future with Time Dilation! The Universe Effect Published on Oct 26, 2015, last accessed Sunday, May 6th, 2018 17:54 PM)

A comet, in a presumed elliptical orbit generated the signal captured by two radios. Wow! was not split by lensing. Here, we have two radios, capturing the signal from a comet moving at X kilometers per second. The frequency shift could be chalked up to nothing more than the Doppler effect. We could plot our radios location, and see if at that time, one radio was moving away from the comet, while the other, due to Earths rotation was moving towards it. Of course, it is the comet sending out the waves, and not Earth. So our recipients would be measuring two different wave patterns. Now, instead of me being gleeful of space-time dilation; the proffered frequency difference is related to wave velocities ratios.
I just stubbed my toe. Someone cancel my dance card, please.

A few observations from the “MathFromTheGut guy”. :

First, the frequency differences you’re talking about are tiny. The relativity portion of those frequency shifts will be miniscule compared to the regular, non relativistic doppler shifts. They really can be ignored.

It really goes back to my MathFromTheGut proof of the Pythagorean theorem. The actual H frequency is about 1420.4, not the rounded 1420 MHz as you mention. This means that these two measurements are off by about .05 MHz out of 1420 MHz or about 1 part in 30,000 in different directions.

So, consider a right triangle whose hypotenuse has a length of 30,000. And its SHORT leg has a length of 1. The length of that other leg (VERY close to 30,000) compared to the hypotenuse tells us how much time is slowing down in the hydrogen’s frame of reference compared to the observer. The difference between those leg lengths can be approximated very well as the contribution of the short leg to the hypotenuse’s length. (Review my video if you don’t follow what I’m talking about.)

The contribution of the short leg to the hypotenuse’s length is proportional to its length (1), and to the ratio of that leg’s length divided by the hypotenuse’s length, or 1/30,000. So, this leg contributes 1/30,000th of a unit to a hypotenuse that is 30,000 units long. In other words it affects the hypotenuse’s length by a multiplicative FACTOR of (1/30,000)^2

Conversely, the regular non-relativsitic Doppler effect changes the frequency by a factor of 1 part in 30,000 or 30,000 times more than the relativistic effect! So we really should completely ignore the relativistic effect here.

Doing this the less intuitive way, non MathFromTheGut way…

Setting B (beta) equal to V/C or 1/30,000 our relativistic doppler shift factor becomes

sqrt( (1-B) / (1+B)) = 1 – B = 1 x 3.3333e-05

Conversely, the conventional Doppler shift factor would be…

1 – B = 1 x 3.3333e-05

In other words, the exact same answer to that many decimal places.

Note a B of 1/30,000 –> a velocity of 1/30,000th the speed of light or only 10 kilometers/sec.

MathFromTheGut wants us to know that all values are approximate!

Yes. Actually that helped a lot!

Learn more about MathFromTheGut:

Where you get to learn Proof of the Pythagorean Theorem in Two Blinks!!

Firstly, it makes the doppler answer the “correct” (if not more obvious) answer.

Secondly, if I clung to relativity – the very small number elucidated speaks volumes of just how stiff space-time is.

I was counting on that either number was correct, despite 1420.4 being the “actual” H frequency. I didn’t think that both signals could have been time shifted. And now I do.

It is now obvious since neither reported signal were mid-point H frequency.

Thank you, MathFromTheGut guy, for the correction on the actual H frequency!

I looked up the reference to a few more decimal points, instead of leaning on Atal.
Here it is, below, and citing a few references herein:

The wiki version shows;
1420405751.7667±0.0009 Hz,[2]

Wikipedias citation is: Dupays, Arnaud; Beswick, Alberto; Lepetit, Bruno; Rizzo, Carlo (August 2003). “Proton Zemach radius from measurements of the hyperfine splitting of hydrogen and muonic hydrogen” (PDF). Physical Review A. 68 (5). arXiv:quant-ph/0308136 . Bibcode:2003PhRvA..68e2503D. doi:10.1103/PhysRevA.68.052503.

citation is also found here:

An open source publication can be found, here:

I’ve put my dancing shoes back on. Don’t worry. “Can you please tell her that mama found her red shoe? She was so worried about that shoe…” -Gravity, scientist Ryan Stone to Astronaut Matt Kowalski (Cuarón, Alfonso, et al. Gravity. Warner Bros. Pictures, 2013.)

I bet you that the Vt was 10 km/s

Accessing the WOW paper, Hydrogen Clouds from Comets 266/P Christensen and P/2008 Y2 (Gibbs) are Candidates for the Source of the 1977 “WOW” Signal, – accessed on May 6, 2018, 19:48) we can cite:

266P/Christensen was 3.8055 AU from Earth and moving at a radial velocity of +13.379 km/s; and P/2008 Y2 (Gibbs) was 4.406 AU from Earth and moving at a radial velocity of +19.641 km/s.

The authors data came from: The International Astronomical Union Minor Planet Center, Database: MPEC 2009- A03 P/2008 Y2 (Gibbs); MPEC 2008-U27 266P/Christensen. accessed on 21 Nov. 2015

10 km/s does co-relate with 13.379 km/s

Calculating the percentage difference we get a 28.9 percent difference.

I may have mistakenly ascribed the doppler shift calculation to a comet velocity, without adjustment.

Perhaps I should note a simpler non-geometry math calculation of:

Earth Velocity (30 km/s) – 10 km/s (doppler shift calculated) = 20 km/s

Which is a number that is eerily close to the radial velocity reported of Gibbs, at 19.641 km/s

tap tap tap. tappidy tapp tapp. Now thats’ tap-dancing!

Editor’s Note: The expansion of the universe, presumably caused by dark energy, can happen at the speeds approaching that of the light and can even exceed the speed of light. This does not violate Albert’s Einstein’s speed limit. Because expansion of the universe is not caused by moving away of galaxies. Instead, new space gets created in between. Like it happened with inflation during he early part of universe’s life when space expanded by orders of magnitude within a short span of time. Sorry Mr. Einstein, you cannot issue a speeding ticket !

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let there be light

by Dave Skitt

let there be light

Let there be light! And it was good.

You may believe from the title that I will be writing about the beginning of the universe, some formula for the speed of light or my first night out with some new telescope or EAA camera gizmo. Well, I am not. Or not completely. As Observatory Chair, I usually stick to topics about the observatory itself.

My initial inspiration for the title comes from the fact that the Simpson observatory now has an awesome set of four, bright white LED work lights. These light strips were expertly installed up in the roof rafters by creative board member Gene Allen.

The need for some form of work lighting has been known and chatted about for quite some time as we have been taking strides to improve the observatory and its equipment. Those working under the closed roof were frequently short on available light and cursed the inadequate light producers they may have brought along with them.

So, one recent night, while Gene Allen, Rex Parker, Tom Swords, Larry Kane, Jennifer Skitt and I were tinkering with the Hastings/Mewlon alignment, it was decided to finally remedy the lighting shortcomings. In order to use the lights, there are two corded plugs that drop down from the rafters to plug into 110vac outlets located on the north and south ends of the eastern wall. Just be sure to remove the plugs and stow the cords back up in the rafters before moving/opening the roof.

The results, shown in the panoramic photos of the entire observatory, are dramatic. You can clearly see everything. Thanks Gene!

Speaking of the Hastings/Mewlon alignment, thanks to Rex Parker for acquiring the fully adjustable ADM plate for the Mewlon base. We now have both scopes pointing at the same object in the sky. And, in the process, we managed to bring the Mewlon eyepiece height down to a more comfortable position. This will go a long way in making the Mewlon more pleasurable to use.

Now, on to the inference about first light. Yes, AAAP has recently acquired two new EAA video cameras. The first is a Starlight Express Ultrastar-C installed on the Explore Scientific refractor in place of the Mallimcam camera. The second is a ZWO ASI294MC Pro installed on the Mewlon scope. First light for the new cameras was on May 23rd with the assistance of Rex Parker, Gene Allen, Tom Swords and myself. Initial impressions of the images were highly positive, with the understanding that the results will only get better as our experience with these devices and software grows. Stay tuned for updates.

So there you have it. I spoke about new light, aligned light and first light and it wasn’t too technical.

Looking East

Looking East

Looking West

Looking West

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Thunderbird and the seven girls

by Ted Frimet


and the seven girls

Thunderbird and his seven girls grew up to know dark skies. Their view was a serene night time walk-about. Every evening, they would naked eye peer into the blackness. Then they would bear witness to the sacred agreement.

Each passing Spring evening, Hehaka the Elk would shelter under Canhasa the Red Willow. And the seven girls awed with wonder seeing them together. If only I were the Elk, and my sisters were the Willow, mused one of seven. I would then know what lay beyond the Earths horizon.

Thunderbird taught the seven girls their relationship with the night sky. He reminded them not to be indifferent to it. They were taught to embrace Oceti the Fireplace and Mato Tipila the Bear’s Lodge, rising in the East. And remember well to say their evening goodbyes to Thunderbird and the Elk, in the setting West.

Time passed, and Earth became a smaller place. Newcomers came to the land where Thunderbird and the seven girls lived. And for awhile, they shared their skies with the newcomers. It was a sharing, after all, gifted from a people that knew the night stories and spoke often of their responsibility to sky and earth.

Over the passing of many seasons, the newcomers commitment was not honored. And Thunderbird grew old and tired. To Tun Win, the Blue Birth Woman, whispered into the ear of Thunderbird. She softly spoke to him his real name. “Wakinyan”, she said. Now gifted with the knowledge of his true nature, Wakinyan, dove from the North and descended into the West, never to be seen again.

The seven girls were troubled. Why, To Tun Win, did you whisper the true name to our father, Thunderbird? He is now gone from us, forever. To Tun Win told the seven girls that they needed to understand the world as being deeply interconnected. That they, the people and the few they privileged, were held accountable to sky and earth. And that the newcomer’s lights’ casted an ugly gray hue.

Wearily, To Tun Win told the seven girls that she longed for seeing Anpo Wicanhpi Sunkaku, the Younger Brother of Morning Star. And to do so with her naked eyes. The gray hue of scattered light kept her from Anpo, she said.

Now forlorn, To Tun Win gathered the seven girls about her. She spoke hesitantly of the passed time for dark skies. She said quietly, “Our reservation has no boundary”. We shared our imaginary lines in the sky. We showed them where we store our history. Where we hunt and where we fish. And despite what stories we tell, we have no real protection.

The newcomers continue to bring the scattered lights. Thunderbird, she exclaimed, is gone forever. He did not protect the night sky. However, you can bring me back my Anpo Wicanhpi Sunkaku.

“How, shall we?”, the sisters asked. Once again To Tun Win whispered softly. Although she spoke to all, each sister felt as if To Tun Win whispered into only her ear.

You must reach out to the seven lands of Mother Earth. You must teach all newcomers. Remind them of their interconnectedness of Sky and Earth. Then they too will know the nightly whisper of To Tun Win. Until the darkness comes back to me, they will only know the story of Thunderbird.

Remember the darkness of the night sky, and pay homage to this relationship. Understand the interconnectedness of the whole World, below and above. Know that you have no higher sovereign authority than to grant, protect, and preserve the night sky.

When you turn off the lights, you unite mother and sun.

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From the human eye to AI

by Prasad Ganti

From the human eye to AI

It all started with humans observing points of light in the sky with their naked eyes. The quest to understand our planet earth, our solar system, our galaxy, and ultimately the whole universe. Astronomy grew from such humble beginnings. Aided by imagination, technology inventions, growth in science, we have come a long way. And astronomy today is no longer just looking at the sky with the naked eye. Although that task still forms the basis of human curiosity.

Some material for this article has been taken from the book “The Big Bang” by Simon Singh. This book had a great impact on me by laying down the astronomy timeline very clearly. The AI (Artificial Intelligence) part is an addition of my 2 cents. Observation of the skies with naked eye reached its peak with the Danish astronomer Tyco Brahe’s gathering a lot of experimental data which Johannes Kepler used to firmly establish the sun centric model of our solar system with the planets going around. Planets up to Saturn were known and distinguished from stars which stayed relatively fixed in the skies. Comets were known as well.

Hans Lippershey, a Flemish spectacle maker invented the telescope in 1608, which Galileo Galilei made use of. Galileo first observed that Jupiter had four moons and also discovered the rings of Saturn. The telescope extended man’s vision to distant skies. Telescopes became more and more powerful as time went by. Also enabling seeing near objects in much greater detail.

After Galileo, William Herschel was a great user of the telescope. He discovered Uranus, who was the father of Saturn and grand father of Jupiter in Greek mythology. Other than the planets and the stars, there were hazy objects called nebulae. Charles Messier compiled a catalog of 103 nebulae in 1781. These are distant objects, like M31 (31st object in Messier catalog) which is Andromeda, now known as a separate galaxy.

The next milestone came when John Herschel, son of William, started photographing stars. This let the pictures to be analyzed by different teams at future points in time. John Goodricke discovered the Cepheid stars which have variable brightness. Because they go through contraction and expansion cycles. Henrietta Leavitt found a relationship between the period of fluctuation and the apparent brightness by collecting data from a group of Cepheids in the Magellanic cloud. A team of astronomers found the distance to one Cepheid. Henrietta’s graph was used to calculate distances to other Cepheids. Thus Cepheids are known as standard candles.

Edwin Hubble has been the first astronomer to find Cepheids outside the Milky Way and thereby measure the distance to our neighboring Galaxy, namely the Andromeda Galaxy. Finding Cepheids in distant galaxies was not possible. Astronomers made an assumption that the brightest star in all the galaxies have the same absolute brightness. By comparing the apparent brightness, a Galaxy’s distance could be measured.

After Isaac Newton used a prism to split the sunlight into rainbow colors, Joseph Von Fraunhofer, Robert Bunsen and Gustav Kirchhoff built a spectroscope for measuring wavelengths of lights emitted by an object. Each element has its own characteristic emission and absorption line. A great achievement of this technique has been the discovery of an absorption line in sunlight which did not match any element on the earth. It was called Helium. This technique is used to find the contents of a remote object and its atmosphere.

William Herschel accidentally discovered infrared rays. He placed a thermometer in different colors produced by a prism. He tried to measure the temperature of something invisible beyond the red light. He found that portion to be the hottest. Heat radiation is now what is known as infrared rays. In the last half century or so, astronomy galloped to detect other parts of the electromagnetic spectrum, ie. radio waves, infrared waves, ultraviolet waves, x-rays, gamma rays etc. Different telescopes detect different parts of the electromagnetic spectrum. Astronomical objects in the Universe emit more than light. In fact, the complete story of an object can be constructed by detecting emissions at various frequencies.

Radio telescopes began with the accidental discovery of a Bell Labs engineer named Karl Jansky. A radio telescope is set of radio antennas connected to a radio receiver receiving. It does not resemble an optical telescope in any way. Bell Labs also contributed to Astronomy with another accidental discovery of what now is known as cosmic background radiation at microwave frequencies.

Most recent trend has been the discovery of exoplanets. Planets which are outside of our solar system and which can harbor life. Obviously the stars cannot harbor any life. The exoplanetshave to be discovered indirectly, by the dimming of the light from its parent star, or by the wobble it causes to its parent star. It means measuring very subtle variations in light and movement and interpreting the data. This is where AI comes into picture. Recent trends in machine learning involves taking vast amount of data and finding hidden patterns. Quicker than what a human being could have done. In fact with Google’s help, some exoplanets were found using the gathered data. This bodes well for astronomy.

Telescopes have moved to space to avoid the terrestrial disturbances. While bigger and bigger ones get built on the ground. Reams of data is being collected and analyzed by the computers. Big data and AI are coming to the aid. Newer discoveries are being made. We certainly have come a long way from the days of gazing at the night skies or peeping into an optical telescope.

Posted in June 2018, Sidereal Times | Tagged | Leave a comment


compiled by Arlene & David Kaplan

Insight mission -BBC

Insight mission -BBC

InSight Diary: Mars mission ready to rumble
The InSight mission will investigate the interior structure and composition of Mars. Prof Tom Pike from Imperial College London is part of the science team on the US-led InSight mission to Mars. His group has supplied seismometers that will enable the Nasa lander to detect “Marsquakes”, which should reveal…more

Many universes -BBC

Many universes -BBC

Prof Stephen Hawking’s final paper resolves universe paradox
Prof Stephen Hawking’s final research paper suggests that our Universe may be one of many similar to our own. The theory resolves a cosmic paradox of the late physicist’s own making. It also points a way forward…more

2001: A Space Odyssey - NYT

2001: A Space Odyssey – NYT

‘2001: A Space Odyssey’ Is Still the ‘Ultimate Trip’
In honor of its 50th anniversary it is being rereleased at the Cannes Film Festival. Stanley Kubrick’s masterpiece encourages us to reflect again on where we’re coming from and where we’re going…more

The Big Falcon Rocket (BFR)

The Big Falcon Rocket (BFR) – SpaceX

SpaceX flies ‘lessons learned’ rocket
The California rocket company SpaceX has conducted what is arguably its most important launch to date. Flying out of Florida, the firm’s Falcon-9 vehicle lifted a standard telecommunications satellite for Bangladesh into orbit. But the booster incorporated everything SpaceX has so far learnt …more

Calendar of astronomy/space events
Sync your calendar with the solar system…more

A view of the Milky Way and neighboring galaxies, containing more than a billion stars, released by the European Space Agency’s Gaia mission.CreditESA/Gaia/DPAC

A view of the Milky Way and neighboring galaxies, containing more than a billion stars, released by the European Space Agency’s Gaia mission.CreditESA/Gaia/DPAC

Gaia’s Map of 1.3 Billion Stars Makes for a Milky Way in a Bottle
Call it a galaxy in a bottle….more

Illustraion: 2004 EW95 orbits four billion kilometres from Earth

Illustraion: 2004 EW95 orbits four billion kilometres from Earth

Lonely asteroid tells Solar System story
Researchers have observed the first object of its kind – a carbon-rich asteroid in the Kuiper Belt…more

Nasa provided this computer-generated image of the helicopter's design

Nasa provided this computer-generated image of the helicopter’s design

Nasa will send helicopter to Mars to test other worldly flight
Nasa is sending a helicopter to Mars, in the first test of a heavier-than-air aircraft on another planet…more

Illustraion: 2004 EW95 orbits four billion kilometres from Earth

Illustraion: 2004 EW95 orbits four billion kilometres from Earth

Lonely asteroid tells Solar System story
Researchers have observed the first object of its kind – a carbon-rich asteroid in the Kuiper Belt…more

MACS1149-JD1 was originally found by Hubble, but was analysed using the VLT and Alma The team is not quite finished

MACS1149-JD1 was originally found by Hubble, but was analysed using the VLT and Alma
The team is not quite finished

Scientists detect oxygen legacy of first stars
They observed it in a galaxy of stars that existed just 500 million years after the Big Bang…more

In pictures: Astronomy Photographer of the Year 2017
The winning images from this year’s competition have now been announced, with Artem Mironov’s vibrant clouds of dust and gas in the Rho Ophiuchi Cloud Complex scooping first place…more

An illustration of a grey/white asteroid on a starfield

An illustration of a grey/white asteroid on a starfield

‘Permanent’ interstellar visitor found
An asteroid in Jupiter’s orbit may have come from outside our Solar System, according to a new study…more

The satellites were assembled in Europe by Airbus

The satellites were assembled in Europe by Airbus

Grace mission launches to weigh Earth’s water
The Grace satellites are replacing a pair of highly successful spacecraft that stopped working last year…more

Charles Duke is the youngest person to have walked on the moon

Charles Duke is the youngest person to have walked on the moon

Moon walking: Ex-Nasa astronauts describe lunar experience
The last US mission to the Moon, Apollo 17, blasted off shortly before midnight on 7 December 1972. Its crew spent three days on the lunar surface, collecting samples and conducting experiments…more

Posted in June 2018, Sidereal Times | Tagged , | Leave a comment